The strong magnetic field of neutron stars is intimately coupled to the observed temperature
and spectral properties, as well as to the observed timing properties (distribution of spin …

Young and rotation-powered neutron stars (NSs) are commonly observed as rapidly-
spinning pulsars. They dissipate their rotational energy by emitting pulsar wind with …

Simulating the long-term evolution of temperature and magnetic fields in neutron stars is a
major effort in astrophysics, having significant impact in several topics. A detailed …

Neutron stars are compact and dense celestial objects that offer the unique opportunity to
explore matter and its interactions under conditions that cannot be reproduced elsewhere in …

Neutron stars harbor extremely strong magnetic fields within their solid outer crust. The
topology of this field strongly influences the surface temperature distribution and, hence, the …

We perform the first 3D fully coupled magneto-thermal simulations of neutron stars
(including the most realistic background structure and microphysical ingredients so far) …

Motivated by the recent detection of ultralong-period radio transients, we investigate new
models of coherent radio emission via low-altitude electron–positron pair production in …

We report the radio and high-energy properties of a new outburst from the radio-loud
magnetar 1E 1547.0− 5408. Following the detection of a short burst from the source with …

Magnetic field evolution in neutron-star crusts is driven by the Hall effect and Ohmic
dissipation, for as long as the crust is sufficiently strong to absorb Maxwell stresses exerted …

Magnetars exhibit a variety of transient high-energy phenomena in the form of bursts,
outbursts, and giant flares. It is a common belief that these events originate in the sudden …